. (2009) Stellar and galactic environment survey (SAGE). Astrophysics and Space Science, Vol.320 (No.1-3). pp. 231-238. ISSN 0004-640X

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Abstract

This paper describes a proposed high resolution soft X-ray and Extreme Ultraviolet (EUV) spectroscopy mission to carry out a survey of Stellar and Galactic Environments (SAGE). The payload is based on novel diffraction grating technology which has already been proven in a sub-orbital space mission and which is ready to fly on a satellite platform with minimal development. Much of the technical detail of the instrumentation has been reported elsewhere and we concentrate our discussion here on the scientific goals of a SAGE base-line mission, demonstrating the scientific importance of high resolution spectroscopy in the Extreme Ultraviolet for the study of stars and the local interstellar medium.

Item Type:	Journal Article
Subjects:	Q Science > QB Astronomy Q Science > QC Physics
Divisions:	Faculty of Science > Physics
Library of Congress Subject Headings (LCSH):	Ultraviolet spectroscopy, Astronomical instruments, Interstellar matter
Journal or Publication Title:	Astrophysics and Space Science
Publisher:	Springer
ISSN:	0004-640X
Date:	April 2009
Volume:	Vol.320
Number:	No.1-3
Number of Pages:	8
Page Range:	pp. 231-238
Identification Number:	10.1007/s10509-008-9792-9
Status:	Peer Reviewed
Publication Status:	Published
Access rights to Published version:	Restricted or Subscription Access
Conference Paper Type:	Paper
Title of Event:	Conference on Network for Ultra Violet Astronomy
Type of Event:	Conference
Location of Event:	Madrid, Spain
Date(s) of Event:	JUN, 2007
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URI:	http://wrap.warwick.ac.uk/id/eprint/28354

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